The structure and stability of the first generation stars of M. and M. on the zero-age main sequence.

1978
İbrahim, Aysel

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Evolutionary study of a rotating 20M. star with a chemical composition appropriate for the Large Magellanic Cloud (LMC) has been carried out starting from the threshold of stability through the gravitational contraction phase, approach to the main-sequence, on the hydrogen burning phase, upto the point at which 61% of hydrogen was consumed in the central region of the star. During evolution mixing due to diffusion has been taken into account. As a consequence of such a mixing it has been shown that the atmo...
Citation Formats
A. İbrahim, “The structure and stability of the first generation stars of M. and M. on the zero-age main sequence.,” Ph.D. - Doctoral Program, Middle East Technical University, 1978.